Solar Cycle Dynamics

Solar Cycle Dynamics is a theoretical framework that describes the temporal evolution and physical mechanisms governing the periodic variations in solar magnetic activity, including sunspot formation, polarity reversals, and solar irradiance changes, over an approximately eleven-year cycle.

1.1K

Publications

55.9K

Citations

1.9K

Authors

704

Institutions

Publications per year

2017–2026

234

Authors

1.9K

  1. KL
    Kejun Li

    National Astronomical Observatories, China

    20 publications · 672 citations

    17

    h-index

  2. MD
    Mausumi Dikpati

    NSF NCAR High Altitude Observatory, United States

    18 publications · 1.6K citations

    16

    h-index

  3. PA
    Peter A. Gilman

    NSF NCAR High Altitude Observatory, United States

    14 publications · 1.3K citations

    14

    h-index

  4. ZD
    Zhanle Du

    Chinese Academy of Sciences, China

    14 publications · 312 citations

    13

    h-index

  5. PC
    Paul Charbonneau

    Université de Montréal, Canada

    12 publications · 1.8K citations

    12

    h-index

1–5 of 1.9K

Venues

  1. The Astrophysical Journal

    ApJ · 133 publications · 11.2K citations

    54

    h-index

  2. Solar Physics

    171 publications · 8.1K citations

    52

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 78 publications · 5K citations

    42

    h-index

  4. Astronomy and Astrophysics

    62 publications · 3.1K citations

    32

    h-index

  5. Geophysical Research Letters

    42 publications · 3.3K citations

    30

    h-index

1–5